Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic clouds

Authors :: Tisserand, Patrick
Le Guillou, L
Afonso, C
Albert, J N
Anderson, J
Ansari, R
Aubourg, E
Bareyre, P
Beaulieu, J.-P
Charlot, X
Coutures, C
Ferlet, R
Fouque, P
Glicenstein, J F
Goldman, B
Gould, A
Graff, D.
Gros, M
Haissinski, J
Hamadache, C.
de Kat, J
Lasserre, T
Lesquoy, E
Loup, C
Magneville, C
Marquette, J B
Maurice, E
Maury, A.
Milsztajn, A
Moniez, M
Palanque-Delabrouille, N
Perdereau, O
Rahal, Y R
Rich, J
Spiro, M
Vidal-Madjar, A
Vigroux, L
Zylberajch, S
Tisserand, Patrick
Le Guillou, L
Afonso, C
Albert, J N
Anderson, J
Ansari, R
Aubourg, E
Bareyre, P
Beaulieu, J.-P
Charlot, X
Coutures, C
Ferlet, R
Fouque, P
Glicenstein, J F
Goldman, B
Gould, A
Graff, D.
Gros, M
Haissinski, J
Hamadache, C.
de Kat, J
Lasserre, T
Lesquoy, E
Loup, C
Magneville, C
Marquette, J B
Maurice, E
Maury, A.
Milsztajn, A
Moniez, M
Palanque-Delabrouille, N
Perdereau, O
Rahal, Y R
Rich, J
Spiro, M
Vidal-Madjar, A
Vigroux, L
Zylberajch, S
Source :: Astronomy and Astrophysics
Publication Year :: 2007
Abstract: Aims. The EROS-2 project was designed to test the hypothesis that massive compact halo objects (the so-called "machos") could be a major component of the dark matter halo of the Milky Way galaxy. To this end, EROS-2 monitored over 6.7 years 33 × 106 star

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